Abstract
Despite interest as early as in the 1880s, it was not until 1953 that Tokimi Tsujita (Seikai Fisheries Research Laboratory, Japan) was able to carefully collect and describe the matrix of microorganisms embedded in suspended organic matter (Tsujita, J Oceanogr Soc Jpn 8:1–14, 1953) that today we call marine snow. Subsequent studies reported that marine snow consisted of phytoplankton, small zooplankton, fecal material, and other particles (Nishizawa et al., Bull Fac Fish, Hokkaido Univ. 5:36–40, 1954). Across the ocean, Riley (Limnol Oceanogr 8:372–381, 1963) called this material “organic aggregates” which in addition to the organic material included nonliving material that was a “substrate for bacterial growth.” More than a decade later, Silver et al. (Science 201:371–373, 1978) quantified the abundance of marine snow, and its contribution to the total community in situ, and showed that marine snow particles were “metabolic hotspots,” with concentrations of microorganisms 3–4 orders of magnitude greater than those in the surrounding seawater. Alldredge and Cohen (Science 235:689–691, 1987) emphasized the importance of marine snow as unique chemical and physical microhabitats. The importance of transparent exopolymer particles (TEP), which form the matrix that embeds the individual component particles of marine snow, were described and quantified in the early 1990s (Alldredge et al., Deep-Sea Res I 40: 1131–1140, 1993; Passow and Alldredge, Mar Ecol Prog Ser 113:185–198, 1994; Passow et al., Deep-Sea Res Oceanogr Abstr 41:335–357, 1994).
The long-held belief that marine snow was both a specialized habitat and potential food source for those living in the deep ocean was also demonstrated at that time (Silver and Gowing, Prog Oceanogr 26:75–113, 1991). More recently it was confirmed that marine snow does indeed contribute significantly to the metabolism of the deep sea and provides hotspots of microbial diversity and activity at depth (e.g., Burd et al., Deep-Sea Res II 57:1557–1571, 2010; Bochdansky et al., Sci Rep 6:22633, 2016). Moreover, marine snow is now considered a transport vehicle for its biota and associated particulate matter (Volk and Hoffert, The carbon cycle and atmospheric CO: natural variations archean to present. American Geophysical Union, Washington, D.C., pp. 99–110, 1985; Alldredge and Gotschalk, Limnol Oceanogr 33:339–351, 1988). Rapidly sinking marine snow is important in the marine carbon cycle as it is responsible for vertical (re)distribution and remineralization of carbon. The transport of carbon from the surface to the deep sea is known as the “biological carbon pump” (De La Rocha and Passow, Deep Sea Res II 54:639–658, 2007; De La Rocha and Passow, Treatise on Geochemistry. Vol. 8, Elsevier, Oxford, 2014). This pump, which leads to the uptake and sequestration of atmospheric CO2 (e.g., Volk and Hoffert, The carbon cycle and atmospheric CO: natural variations archean to present. American Geophysical Union, Washington, D.C., pp. 99–110, 1985; Finkel et al., J Plankton Res 32:119–137, 2010; Zetsche and Ploug, Mar Chem 175:1–4, 2015), also plays an important role in the biogeochemical cycling of elements (e.g., Quigg et al., Nature 425:291–294, 2003; Quigg et al., Proc R Soc: Biol Sci 278:526–534, 2011). How climate change will change these processes is the subject of intense interest but beyond the scope of this chapter.
“I see always the steady, unremitting, downward drift of materials from above, flake upon flake, layer upon layer — a drift that has continued for hundreds of millions of years, that will go on as long as there are seas and continents. For the sediments are the materials of the most stupendous snowfall the earth has ever seen….” (from Rachel Carson, The Sea Around Us, 1951)
“Marine snow is a nearly ubiquitous phenomenon in oceanic waters. The individual particles of marine snow are often fragile, difficult to sample intact, and provide distinctive microenvironments that support unique biological, chemical, and physical processes.” (from Mary Silver 2015)
“Marine snow formation, incorporation of oil, and subsequent gravitational settling to the seafloor (i.e., MOSSFA: Marine Oil Snow Sedimentation and Flocculent Accumulation) was a significant pathway for the distribution and fate of oil, accounting for as much as 14% of the total oil released” as a result of the Deepwater Horizon oil spill in the Gulf of Mexico in 2010. (from Daly et al. 2016)
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Acknowledgments
This research was made possible by a grant from the Gulf of Mexico Research Initiative to Quigg (ADDOMEx), Passow (ADDOMEx, ECOGIG, FOMOSA), Daly (C-IMAGE, FOMOSA), Burd (FOMOSA), and Schwing/Hollander (C-IMAGE). Research support was also provided by the University of South Florida Division of Sponsored Research and Florida Institute of Oceanography to Daly and by the Multi-Partner Research Initiative, via the Department of Fisheries and Oceans, Canada, to Passow.
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Quigg, A. et al. (2020). Marine Oil Snow Sedimentation and Flocculent Accumulation (MOSSFA) Events: Learning from the Past to Predict the Future. In: Murawski, S., et al. Deep Oil Spills. Springer, Cham. https://doi.org/10.1007/978-3-030-11605-7_12
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